Open AccessOn the fate of gas in ultraluminous infrared galaxies at low and high redshift
Author(s) -
Trentham Neil
Publication year - 2001
Publication title -
monthly notices of the royal astronomical society
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 2.058
H-Index - 383
eISSN - 1365-2966
pISSN - 0035-8711
DOI - 10.1046/j.1365-8711.2001.04093.x
Subject(s) - physics , astrophysics , luminous infrared galaxy , james clerk maxwell telescope , galaxy , peculiar galaxy , astronomy , galaxy group , star formation , redshift
It is often suggested that the distant galaxies recently identified in 850‐μm surveys with the SCUBA bolometer array on the James Clerk Maxwell Telescope are high‐redshift analogues to local ultraluminous infrared galaxies, based on their similar spectral energy distributions and luminosities. We show that these two populations of objects must differ in at least one fundamental way from each other. This assertion is based on a consideration of the possible fates of gas in the high‐redshift SCUBA galaxies, given the requirement that they most evolve into some subset of the low‐redshift galaxy population with a comoving density of about 10 −4 Mpc −3 . One possibility is that the SCUBA galaxies have similar gas density profiles to local ultraluminous galaxies. If this is the case, then they must derive almost all their power from active galactic nuclei, which appears not to be the case for local ultraluminous galaxies, which are predominantly star‐formation‐powered. Another possibility is that the SCUBA galaxies have more extended gas density profiles than local ultraluminous galaxies. In this case they must be almost all star‐formation‐powered, and much of the star formation in the Universe can happen in these objects. Either way there is a significant difference between the low‐ and high‐redshift populations.